Optical Anisotropy of Nanotube Suspensions Erik K

Total Page:16

File Type:pdf, Size:1020Kb

Optical Anisotropy of Nanotube Suspensions Erik K JOURNAL OF CHEMICAL PHYSICS VOLUME 121, NUMBER 2 8 JULY 2004 Optical anisotropy of nanotube suspensions Erik K. Hobbiea) National Institute of Standards and Technology, Gaithersburg, Maryland 20899 ͑Received 16 January 2004; accepted 7 April 2004͒ A semimacroscopic model of an optically anisotropic nanotube suspension is derived perturbatively from Maxwell’s equations in a dielectric medium. We calculate leading-order expressions, valid in the dilute and semidilute limits, for the intrinsic and form contributions to the complex dielectric tensor in terms of the volume fraction, mean orientation, aspect ratio, optical anisotropy, and optical contrast of the nanotubes. The birefringence and dichroism are derived explicitly to leading order in fluctuations, and the connection with depolarized light scattering is established. The results are generalized to include tube deformation. © 2004 American Institute of Physics. ͓DOI: 10.1063/1.1760079͔ I. INTRODUCTION sions and melts. The approach is reminiscent of the general theory of flow-induced optical anisotropy in dilute polymer It is well known that flow can induce optical anisotropy solutions derived by Onuki and Doi,6 and it expands on a in macromolecular fluids and colloidal suspensions in the previous treatment of depolarized light scattering from car- 1,2 form of birefringence and dichroism. As first demonstrated bon nanotube suspensions.5 We derive general expressions 3 by Peterlin and Stewart, these effects separate naturally into for both the intrinsic and form contributions to the dielectric two distinct parts; an intrinsic contribution arising from the tensor, and we derive leading-order expressions for the bire- orientation of optically anisotropic polymer segments or par- fringence and dichroism. The connection to depolarized light ticles, and a form contribution arising from anisotropy in the scattering is established and the results are generalized to segmental or density correlation function. The experimental include tube deformation. techniques of flow birefringence and flow dichroism have proven to be powerful tools for studying the structural and dynamic properties of flowing polymer melts, polymer solu- II. INTRINSIC CONTRIBUTION tions, and anisotropic suspensions, which in turn has contrib- For a quasistatic suspension of N optically anisotropic uted to recent technological advances in the engineering and nanotubes in an optically isotropic solvent of dielectric con- ␧ flow processing of complex fluids. stant s illuminated by an incident electric field E(r,t) ϭ i(k rϪ␻t) 2ϭ␧ ␻2 2 Recently, carbon nanotubes have emerged as novel ma- E0e • , where k s /c and k points along the terials with potential applications in a host of advanced direction of propagation ͑see Fig. 1͒, the macroscopic dielec- 4 technologies. Nanocomposites engineered from polymers tric tensor can be defined via and carbon nanotubes, for example, offer the promise of ͑ ͒ϭ␧ ͑ ͒ϭ␧ i(k rϪ␻t) ͑ ͒ plastic materials with enhanced structural, thermal, elec- D r,t ˜ •E r,t ˜ •E0e • , 1 ␧ϭ͚3 ␧ tronic, and optical properties. Efficient bulk processing of where the tensor ˜ ␮,␯ϭ1xˆ␮ ␮␯xˆ␯ is homogeneous. If r such composites will depend in part on a detailed under- locates a segment of a nanotube, nˆ(r), then the spatially standing of the response of carbon nanotube suspensions and varying amplitude of the displacement field induced at r is melts to flow. As colloidal particles, nanotubes are also D͑r͒ϭ͕␣ʈnˆ͑r͒nˆ͑r͒ϩ␣Ќ͓1Ϫnˆ͑r͒nˆ͑r͔͖͒ E , ͑2͒ somewhat unique and intriguing, in that they straddle the • 0 interface between semiflexible polymers and microscopic fi- where the local complex dielectric constants ␣ʈ and ␣Ќ arise bers. Given the significant optical contrast between carbon from polarization and absorption along and normal to the nanotubes and most typical polymers, it is reasonable to ex- local symmetry axis of the nanotube, respectively, and 1 is pect that such suspensions will exhibit reasonably strong op- the identity tensor. The parameters ␣ʈ and ␣Ќ appear in the tical anisotropy, making them well-suited to rheo-optical formulas for the depolarized scattering of monochromatic techniques.5 Applied to such novel soft materials, the meth- light from nanotube suspensions.5 Equation ͑2͒ defines a ods of flow birefringence and flow dichroism might offer local dielectric tensor as new physical insight into both fundamental flow-structure ˜␧͑r͒ϭ␣ʈnˆ͑r͒nˆ͑r͒ϩ␣Ќ͓1Ϫnˆ͑r͒nˆ͑r͔͒, ͑3͒ relationships in anisotropic complex fluids, as well as funda- ␧ ϭ␧ mental information about the optical properties and optical when r falls within a tube and ˜ (r) s1 otherwise. Intro- Ϫ anisotropy of the nanotubes themselves. ducing the spatial average ͗˜␧͘ϭV 1͐dr˜␧(r), where V is the In this paper, we present a semimacroscopic calculation sample volume, we obtain the intrinsic part of the dielectric of the complex dielectric tensor of carbon nanotube suspen- tensor ␧ ϭ ␧ ϭ␾ ␣ ϩ␣ Ϫ ͒ ϩ Ϫ␾͒␧ ˜ 0 ͗˜͘ ͓ ʈ͗nˆ lnˆ l͘ Ќ͑1 ͗nˆ lnˆ l͘ ͔ ͑1 s1, a͒Electronic mail: [email protected] ͑4͒ 0021-9606/2004/121(2)/1029/9/$22.001029 © 2004 American Institute of Physics Downloaded 21 Jul 2004 to 129.6.154.32. Redistribution subject to AIP license or copyright, see http://jcp.aip.org/jcp/copyright.jsp 1030 J. Chem. Phys., Vol. 121, No. 2, 8 July 2004 Erik K. Hobbie Multiplying by eϪik"r to remove the harmonic spatial depen- dence and taking the spatial average, this term averages to zero,8 and the first non-vanishing correction to D is thus second order in ␦˜␧(r), being ␦˜␧͑rЈ͒ ͵ Ј ͑ Ј͒ ЈÃ Јϫ ͵ Љ ͑ Ј Љ͒ ЉÃ Љ dr G r,r ␧ dr G r ,r “ “ s • “ “ FIG. 1. A cartoon showing an aligned nanotube suspension. The suspending ␧ medium is of uniform dielectric constant s . The incident field, E0(r,t), is ␦˜␧͑rЉ͒ linearly polarized along the ‘‘slow’’ axis of the suspension. After transmis- ϫ Љ ͑ ͒ ␧ D0 , 8 sion, the polarization is unchanged but the amplitude is attenuated by ab- s • sorption. An incident field linearly polarized along the ‘‘fast’’ axis, or at 90° to the shown scenario, is altered in a similar manner. Light linearly polarized which becomes at an angle between these directions will also emerge attenuated, but with a ␦˜␧͑rЈ͒ ␦˜␧͑rЉ͒ polarization that is elliptical. We seek to calculate the effective dielectric ͵ Ј ͵ Љ ik"rЉ ␧ ͓ Љ Љ dr ␧ dr e ␧ ˜ 0 E0 tensor of the suspension. s • s • • • “ “ ͒ ͑ Ϫٌ͑2͒Љ ͔ ͑ Ј Љ͒ ͓ Ј ЈϪٌ͑2͒Ј ͔ ͑ Ј͒ 1 G r ,r • “ “ 1 G r,r . 9 8 Ϫ Resolving the singularities in the Green’s functions, intro- where ␾ is the volume fraction and ͗nˆ nˆ ͘ϭN 1͚ nˆ nˆ .As l l l l l ducing their Fourier representation, multiplying by eϪik"r in a previous derivation of the light-scattering amplitude,5 we and taking the spatial average, the correction to ˜␧ is neglect contributions of linear and higher order in the differ- 0 ence between the end-to-end vector of the lth nanotube and ͗␦˜␧2͘ 1 ˜␧ ϭ ˜␧ ϩ ͵ dq˜T͑kϪq͒ ˜␧ its body director, nˆ l , which is equivalent to assuming that the 1 ␧2 • 0 ͑2␲͒3 • 0 tubes are nominally straight. The results will be generalized s to include deformation. Ϫqqϩk21 ͫ ͬ, ͑10͒ • q2Ϫ͑kϩi␵͒2 where the tensor III. SPATIAL FLUCTUATIONS ˜ ͑ ͒ϭ ͵ Ϫiq"r͗␦␧͑ ͒ ␦␧͑ ͒͘ ␧2 ͑ ͒ The earlier derivation gives just the leading-order part of T q dre ˜ r • ˜ 0 / s 11 the complex dielectric tensor. In general, there will be is related to the structure factor. Equation ͑10͒ is analogous higher-order contributions arising from the spatial variations to the expression derived by Onuki and Doi6 and is quite ␦˜␧(r)ϭ˜␧(r)Ϫ͗˜␧͘. Following Jackson’s treatment of Ray- general. As derived here, it contains two terms of leigh scattering,7 we obtain these terms perturbatively from O(␦˜␧2/␧2); a higher-order intrinsic correction arising purely the vector wave equation for D, which can be derived from s from mean-square fluctuations and a leading-order form cor- Maxwell’s equations in a dielectric medium. In the harmonic rection involving density correlations identical to that de- approximation in which all fields have a time dependence of ␻ rived in Ref. 6. This result is somewhat intuitive, as one the form ei t, this becomes an inhomogeneous vector Helm- could envision particles lacking any spatial correlation that holtz equation could still alter the polarization of incident light, with the 2ϩ 2͒ ϭϪ Ã Ã͑ Ϫ␧ ͒ ͑ ͒ physical scenario being optically anisotropic particles tooٌ͑ k D “ “ D sE . 5 small to visibly scatter. More quantitatively, for particles Following Jackson,7 the term in parenthesis on the right-hand ͗␦␧ ␦␧ ͘ lacking any segmental correlation ˜ (r)• ˜ (0) ͑ ͒ ␦␧ ␧ ϭ␧ 2 Ϫr2/2␰2 2 3 side of Eq. 5 is written as ˜ (r) D0 / s , where D0 ˜ 0 Ϸlim␰! ͗␦˜␧ ͘e ϰlim␰! ͗␦˜␧ ͘␰ ␦(r), and the second ik"r • 0 0 •E0e . As in scattering theory, a formal solution is then term in Eq. ͑10͒ vanishes, implying that for such ‘‘formless’’ obtained via successive iterations in terms of the Helmholtz ␧ nanotubes the leading-order intrinsic correction to ˜ 0 is sim- Green’s function ply proportional to the mean-square deviation.9 The full ex- ͉ Ϫ Ј͉ Ϫ Ј pression for the dielectric tensor is thus 1 eik r r 1 eiq•(r r ) ͑ Ј͒ϭ ϭ ͵ 2 G r,r 3 dq 2 2 , ͗␦˜␧ ͘ 1 4␲ ͉rϪrЈ͉ ͑2␲͒ q Ϫ͑kϩi␵͒ ␧Ϸ ϩ ϩ ͵ ˜ ͑ Ϫ ͒ ͑ ͒ ˜ ͭ 1 ␧2 ͑ ␲͒3 dqT k q 6 s 2 where the positive infinitesimal ␵ is needed to ensure causal- Ϫqqϩk21 6 ͫ ͬͮ ˜␧ ϩ..., ͑12͒ ity in the displacement field, D(r,t). The first-order correc- • q2Ϫ͑kϩi␵͒2 • 0 tion is ␧ where we have exploited that fact that ˜ 0 is symmetric.
Recommended publications
  • 2.1.5 Stress-Strain Relation for Anisotropic Materials
    ,/... + -:\ 2.1.5Stress-strain Relation for AnisotropicMaterials The generalizedHook's law relatingthe stressesto strainscan be writtenin the form U2, 13,30-32]: o,=C,,€, (i,i =1,2,.........,6) Where: o, - Stress('ompttnents C,, - Elasticity matrix e,-Straincomponents The material properties (elasticity matrix, Cr) has thirty-six constants,stress-strain relations in the materialcoordinates are: [30] O1 LI CT6 a, l O2 03_ a, -t ....(2-6) T23 1/ )1 T32 1/1l 'Vt) Tt2 C16 c66 I The relations in equation (3-6) are referred to as characterizing anisotropicmaterials since there are no planes of symmetry for the materialproperties. An alternativename for suchanisotropic material is a triclinic material. If there is one plane of material property symmetry,the stress- strainrelations reduce to: -'+1-/ ) o1 c| ct2 ct3 0 0 crc €l o2 c12 c22 c23 0 0 c26 a: ct3 C23 ci3 0 0 c36 o-\ o3 ....(2-7) 723 000cqqc450 y)1 T3l 000c4sc5s0 Y3l T1a ct6 c26 c36 0 0 c66 1/t) Where the plane of symmetryis z:0. Such a material is termed monoclinicwhich containstfirfen independentelastic constants. If there are two brthogonalplanes of material property symmetry for a material,symmetry will existrelative to a third mutuallyorthogonal plane. The stress-strainrelations in coordinatesaligned with principal material directionswhich are parallel to the intersectionsof the three orthogonalplanes of materialsymmetry, are'. Ol ctl ct2ctl000 tl O2 Ct2 c22c23000 a./ o3 ct3 c23c33000 * o-\ ....(2-8) T23 0 00c4400 y)1 yll 731 0 000css0 712 0 0000cr'e 1/1) 'lt"' -' , :t i' ,/ Suchmaterial is calledorthotropic material.,There is no interaction betweennormal StreSSeS ot r 02, 03) andanisotropic materials.
    [Show full text]
  • Multidisciplinary Design Project Engineering Dictionary Version 0.0.2
    Multidisciplinary Design Project Engineering Dictionary Version 0.0.2 February 15, 2006 . DRAFT Cambridge-MIT Institute Multidisciplinary Design Project This Dictionary/Glossary of Engineering terms has been compiled to compliment the work developed as part of the Multi-disciplinary Design Project (MDP), which is a programme to develop teaching material and kits to aid the running of mechtronics projects in Universities and Schools. The project is being carried out with support from the Cambridge-MIT Institute undergraduate teaching programe. For more information about the project please visit the MDP website at http://www-mdp.eng.cam.ac.uk or contact Dr. Peter Long Prof. Alex Slocum Cambridge University Engineering Department Massachusetts Institute of Technology Trumpington Street, 77 Massachusetts Ave. Cambridge. Cambridge MA 02139-4307 CB2 1PZ. USA e-mail: [email protected] e-mail: [email protected] tel: +44 (0) 1223 332779 tel: +1 617 253 0012 For information about the CMI initiative please see Cambridge-MIT Institute website :- http://www.cambridge-mit.org CMI CMI, University of Cambridge Massachusetts Institute of Technology 10 Miller’s Yard, 77 Massachusetts Ave. Mill Lane, Cambridge MA 02139-4307 Cambridge. CB2 1RQ. USA tel: +44 (0) 1223 327207 tel. +1 617 253 7732 fax: +44 (0) 1223 765891 fax. +1 617 258 8539 . DRAFT 2 CMI-MDP Programme 1 Introduction This dictionary/glossary has not been developed as a definative work but as a useful reference book for engi- neering students to search when looking for the meaning of a word/phrase. It has been compiled from a number of existing glossaries together with a number of local additions.
    [Show full text]
  • Lecture II Polarization Anisotropy Spectrum
    Lecture II Polarization Anisotropy Spectrum Wayne Hu Crete, July 2008 Damping Tail Dissipation / Diffusion Damping • Imperfections in the coupled fluid → mean free path λC in the baryons • Random walk over diffusion scale: geometric mean of mfp & horizon λD ~ λC√N ~ √λCη >> λC • Overtake wavelength: λD ~ λ ; second order in λC/λ • Viscous damping for R<1; heat conduction damping for R>1 1.0 N=η / λC Power λD ~ λC√N 0.1 perfect fluid instant decoupling λ 500 1000 1500 Silk (1968); Hu & Sugiyama (1995); Hu & White (1996) l Dissipation / Diffusion Damping • Rapid increase at recombination as mfp ↑ • Independent of (robust to changes in) perturbation spectrum • Robust physical scale for angular diameter distance test (ΩK, ΩΛ) Recombination 1.0 Power 0.1 perfect fluid instant decoupling recombination 500 1000 1500 Silk (1968); Hu & Sugiyama (1995); Hu & White (1996) l Damping • Tight coupling equations assume a perfect fluid: no viscosity, no heat conduction • Fluid imperfections are related to the mean free path of the photons in the baryons −1 λC = τ_ where τ_ = neσT a is the conformal opacity to Thomson scattering • Dissipation is related to the diffusion length: random walk approximation p p p λD = NλC = η=λC λC = ηλC the geometric mean between the horizon and mean free path • λD/η∗ ∼ few %, so expect the peaks :> 3 to be affected by dissipation Equations of Motion • Continuity k Θ_ = − v − Φ_ ; δ_ = −kv − 3Φ_ 3 γ b b where the photon equation remains unchanged and the baryons follow number conservation with ρb = mbnb • Euler k v_ = k(Θ + Ψ) − π − τ_(v − v ) γ 6 γ γ b a_ v_ = − v + kΨ +τ _(v − v )=R b a b γ b where the photons gain an anisotropic stress term πγ from radiation viscosity and a momentum exchange term with the baryons and are compensated by the opposite term in the baryon Euler equation Viscosity • Viscosity is generated from radiation streaming from hot to cold regions • Expect k π ∼ v γ γ τ_ generated by streaming, suppressed by scattering in a wavelength of the fluctuation.
    [Show full text]
  • Cosmic Microwave Background
    1 29. Cosmic Microwave Background 29. Cosmic Microwave Background Revised August 2019 by D. Scott (U. of British Columbia) and G.F. Smoot (HKUST; Paris U.; UC Berkeley; LBNL). 29.1 Introduction The energy content in electromagnetic radiation from beyond our Galaxy is dominated by the cosmic microwave background (CMB), discovered in 1965 [1]. The spectrum of the CMB is well described by a blackbody function with T = 2.7255 K. This spectral form is a main supporting pillar of the hot Big Bang model for the Universe. The lack of any observed deviations from a 7 blackbody spectrum constrains physical processes over cosmic history at redshifts z ∼< 10 (see earlier versions of this review). Currently the key CMB observable is the angular variation in temperature (or intensity) corre- lations, and to a growing extent polarization [2–4]. Since the first detection of these anisotropies by the Cosmic Background Explorer (COBE) satellite [5], there has been intense activity to map the sky at increasing levels of sensitivity and angular resolution by ground-based and balloon-borne measurements. These were joined in 2003 by the first results from NASA’s Wilkinson Microwave Anisotropy Probe (WMAP)[6], which were improved upon by analyses of data added every 2 years, culminating in the 9-year results [7]. In 2013 we had the first results [8] from the third generation CMB satellite, ESA’s Planck mission [9,10], which were enhanced by results from the 2015 Planck data release [11, 12], and then the final 2018 Planck data release [13, 14]. Additionally, CMB an- isotropies have been extended to smaller angular scales by ground-based experiments, particularly the Atacama Cosmology Telescope (ACT) [15] and the South Pole Telescope (SPT) [16].
    [Show full text]
  • Physics of the Cosmic Microwave Background Anisotropy∗
    Physics of the cosmic microwave background anisotropy∗ Martin Bucher Laboratoire APC, Universit´eParis 7/CNRS B^atiment Condorcet, Case 7020 75205 Paris Cedex 13, France [email protected] and Astrophysics and Cosmology Research Unit School of Mathematics, Statistics and Computer Science University of KwaZulu-Natal Durban 4041, South Africa January 20, 2015 Abstract Observations of the cosmic microwave background (CMB), especially of its frequency spectrum and its anisotropies, both in temperature and in polarization, have played a key role in the development of modern cosmology and our understanding of the very early universe. We review the underlying physics of the CMB and how the primordial temperature and polarization anisotropies were imprinted. Possibilities for distinguish- ing competing cosmological models are emphasized. The current status of CMB ex- periments and experimental techniques with an emphasis toward future observations, particularly in polarization, is reviewed. The physics of foreground emissions, especially of polarized dust, is discussed in detail, since this area is likely to become crucial for measurements of the B modes of the CMB polarization at ever greater sensitivity. arXiv:1501.04288v1 [astro-ph.CO] 18 Jan 2015 1This article is to be published also in the book \One Hundred Years of General Relativity: From Genesis and Empirical Foundations to Gravitational Waves, Cosmology and Quantum Gravity," edited by Wei-Tou Ni (World Scientific, Singapore, 2015) as well as in Int. J. Mod. Phys. D (in press).
    [Show full text]
  • Glossary of Materials Engineering Terminology
    Glossary of Materials Engineering Terminology Adapted from: Callister, W. D.; Rethwisch, D. G. Materials Science and Engineering: An Introduction, 8th ed.; John Wiley & Sons, Inc.: Hoboken, NJ, 2010. McCrum, N. G.; Buckley, C. P.; Bucknall, C. B. Principles of Polymer Engineering, 2nd ed.; Oxford University Press: New York, NY, 1997. Brittle fracture: fracture that occurs by rapid crack formation and propagation through the material, without any appreciable deformation prior to failure. Crazing: a common response of plastics to an applied load, typically involving the formation of an opaque banded region within transparent plastic; at the microscale, the craze region is a collection of nanoscale, stress-induced voids and load-bearing fibrils within the material’s structure; craze regions commonly occur at or near a propagating crack in the material. Ductile fracture: a mode of material failure that is accompanied by extensive permanent deformation of the material. Ductility: a measure of a material’s ability to undergo appreciable permanent deformation before fracture; ductile materials (including many metals and plastics) typically display a greater amount of strain or total elongation before fracture compared to non-ductile materials (such as most ceramics). Elastic modulus: a measure of a material’s stiffness; quantified as a ratio of stress to strain prior to the yield point and reported in units of Pascals (Pa); for a material deformed in tension, this is referred to as a Young’s modulus. Engineering strain: the change in gauge length of a specimen in the direction of the applied load divided by its original gauge length; strain is typically unit-less and frequently reported as a percentage.
    [Show full text]
  • Advanced Measurements of Silicon Carbide Ceramic Matrix Composites
    INL/EXT-12-27032 Advanced Measurements of Silicon Carbide Ceramic Matrix Composites David Hurley Farhad Fazbod Zilong Hua Stephen Reese Marat Khafizov August 2012 The INL is a U.S. Department of Energy National Laboratory operated by Battelle Energy Alliance DISCLAIMER This information was prepared as an account of work sponsored by an agency of the U.S. Government. Neither the U.S. Government nor any agency thereof, nor any of their employees, makes any warranty, expressed or implied, or assumes any legal liability or responsibility for the accuracy, completeness, or usefulness, of any information, apparatus, product, or process disclosed, or represents that its use would not infringe privately owned rights. References herein to any specific commercial product, process, or service by trade name, trade mark, manufacturer, or otherwise, does not necessarily constitute or imply its endorsement, recommendation, or favoring by the U.S. Government or any agency thereof. The views and opinions of authors expressed herein do not necessarily state or reflect those of the U.S. Government or any agency thereof. INL/EXT-12-27032 Advanced Measurements of Silicon Carbide Ceramic Matrix Composites David Hurley Farhad Farzbod Zilong Hua Stephen Reese Marat Khafizov August, 2012 Idaho National Laboratory Materials Science and Engineering Department Idaho Falls, Idaho 83415 http://www.inl.gov Prepared for the U.S. Department of Energy Office of Nuclear Energy Under DOE Idaho Operations Office Contract DE-AC07-05ID14517 ii iii ABSTRACT Silicon carbide (SiC) is being considered as a fuel cladding material for accident tolerant fuel under the Light Water Reactor Sustainability (LWRS) Program sponsored by the Nuclear Energy Division of the Department of Energy.
    [Show full text]
  • Anisotropic Complex Refractive Indices of Atomically Thin Materials: Determination of the Optical Constants of Few-Layer Black Phosphorus
    materials Article Anisotropic Complex Refractive Indices of Atomically Thin Materials: Determination of the Optical Constants of Few-Layer Black Phosphorus Aaron M. Ross 1, Giuseppe M. Paternò 2 , Stefano Dal Conte 1, Francesco Scotognella 1,2,* and Eugenio Cinquanta 3 1 Dipartimento di Fisica, Politecnico di Milano, Piazza Leonardo da Vinci 32, 20133 Milan, Italy; [email protected] (A.M.R.); [email protected] (S.D.C.) 2 Center for Nano Science and Technology@PoliMi, Istituto Italiano di Tecnologia (IIT), Via Giovanni Pascoli, 70/3, 20133 Milan, Italy; [email protected] 3 Istituto di Fotonica e Nanotecnologie, Consiglio Nazionale delle Ricerche, 20133 Milan, Italy; [email protected] * Correspondence: [email protected]; Tel.: +39-02-2399-6056 Received: 5 November 2020; Accepted: 14 December 2020; Published: 16 December 2020 Abstract: In this work, studies of the optical constants of monolayer transition metal dichalcogenides and few-layer black phosphorus are briefly reviewed, with particular emphasis on the complex dielectric function and refractive index. Specifically, an estimate of the complex index of refraction of phosphorene and few-layer black phosphorus is given. The complex index of refraction of this material was extracted from differential reflectance data reported in the literature by employing a constrained Kramers–Kronig analysis combined with the transfer matrix method. The reflectance contrast of 1–3 layers of black phosphorus on a silicon dioxide/silicon substrate was then calculated using the extracted complex indices of refraction. Keywords: transition metal dichalcogenides; black phosphorus; two-dimensional materials; complex refractive index; Kramers–Kronig analysis 1. Introduction Two-dimensional materials emerged as a promising option for the development of nanoelectronic and optoelectronic devices, due to their peculiar electronic and optical properties.
    [Show full text]
  • Tuning Structural and Magnetic Properties of Fe Oxide Nanoparticles by Specifc Hydrogenation Treatments S
    www.nature.com/scientificreports OPEN Tuning structural and magnetic properties of Fe oxide nanoparticles by specifc hydrogenation treatments S. G. Greculeasa1, P. Palade1, G. Schinteie1, A. Leca1, F. Dumitrache2, I. Lungu2, G. Prodan3, A. Kuncser1 & V. Kuncser1* Structural and magnetic properties of Fe oxide nanoparticles prepared by laser pyrolysis and annealed in high pressure hydrogen atmosphere were investigated. The annealing treatments were performed at 200 °C (sample A200C) and 300 °C (sample A300C). The as prepared sample, A, consists of nanoparticles with ~ 4 nm mean particle size and contains C (~ 11 at.%), Fe and O. The Fe/O ratio is between γ-Fe2O3 and Fe3O4 stoichiometric ratios. A change in the oxidation state, crystallinity and particle size is evidenced for the nanoparticles in sample A200C. The Fe oxide nanoparticles are completely reduced in sample A300C to α-Fe single phase. The blocking temperature increases from 106 K in A to 110 K in A200C and above room temperature in A300C, where strong inter-particle interactions are evidenced. Magnetic parameters, of interest for applications, have been considerably varied by the specifc hydrogenation treatments, in direct connection to the induced specifc changes of particle size, crystallinity and phase composition. For the A and A200C samples, a feld cooling dependent unidirectional anisotropy was observed especially at low temperatures, supporting the presence of nanoparticles with core–shell-like structures. Surprisingly high MS values, almost 50% higher than for bulk metallic Fe, were evidenced in sample A300C. Fe-based nanoparticles (NPs) show remarkable interest in the scientifc community for various applications such as biomedicine (hyperthermia1, targeted drug delivery2, computed tomography and magnetic resonance imaging contrast agents3,4), catalysis5,6, magnetic fuids7, gas sensors8, high-density magnetic storages 9, water treatment and environment protection 10,11.
    [Show full text]
  • Anisotropy and Stress Distribution in Sand
    121 PROC. OF JSCE, No. 212, APRIL, 1973 ANISOTROPY AND STRESS DISTRIBUTION IN SAND By Nobuchika MOROTO* ation of the stress in sand from that in the ideal SYNOPSIS elastic media has been explained by pointing out the following main reasons, (1) the sand adjacent Sand has both inherent and induced anisotropy. to the loaded area at the surface tends to yield The former is produced by sedimentation and even by low stress, (2) the rigidity of sand in- the latter occurs in shear. Degree of the an- creases with depth. The author considers, how- isotropy is evaluated by means of the deforma- ever, the anisotropies of sand may also contribute tion modulus ratio n = Ex/Ez , and the case n <1 to the measured stresses and displacement in is treated. sand. Barden (1963) has made a short remark Deriving the solutions of stress and displace- on an effect of anisotropy on the behaviour of ment in a cross-anisotropic soil, effect of n on sand mass. the stress and surface settlement in sand is ex- Nonlinearity and anisotropy in the behaviour amined. The results show that the stress and of sand are evident. Hasegawa and Sawada (1971) surface settlement tend to increase near the load show, in their paper of stress solutions in non- in case of n<1. This stress increase in plane linear and heterogeneous elastic half space, that strain case is smaller than that in axial sym- problem of material nonlinearity can be treated metry. It can be known that the author's stress as a kind of problem where rigidity varies with solution is not coincidence with Wolf's.
    [Show full text]
  • CMB Temperature and Polarization Anisotropy Fundamentals
    CMB Temperature and Polarization Anisotropy Fundamentals Wayne Hu Center for Cosmological Physics and Department of Astronomy and Astrophysics, University of Chicago, Chicago IL 60637 Abstract. The tremendous experimental progress in cosmic microwave background (CMB) temperature and polarization anisotropy studies over the last few years has helped establish a standard paradigm for cosmology at intermediate epochs and has simultaneously raised questions regarding the physical processes at the two opposite ends of time.What is the physics behind the source of structure in the universe and the dark energy that is currently accelerating its expansion? We review the acoustic phenomenology that forms the cornerstone of the standard cosmological model and discuss internal consistency relations which lend credence to its interpretation. We discuss future milestones in the study of CMB anisotropy that have implications for inflationary and dark energy models.These include signatures of gravitational waves and gravitational lensing in the polarization fields and secondary temperature anisotropy from the transit of CMB photons across the large-scale structure of the universe. 1. INTRODUCTION The pace of discovery in the field of Cosmic Microwave Background (CMB) anisotropy has been accelerating over the last few years. With it,the basic elements of the cosmological model have been falling into place: the nature of the initial seed fluctuations that through gravitational instability generated all of the structure in the universe,and the mixture of matter-energy constituents that drives its expansion. Since even reviews written a scant year ago (e.g. [1,2,3]) seem out of date today,we will focus mainly on the fundamental physical elements that enter into cosmic microwave background observables.
    [Show full text]
  • Oilfield Anisotropy: Its Origins and Electrical Characteristics
    ANISOTROPY ANISOTROPY ANISOTROPY Oilfield Anisotropy: Its Origins and Electrical Characteristics Barbara Anderson Klaus Helbig Ian Bryant Consultant Martin Lüling Hannover, Germany Brian Spies Ridgefield, Connecticut, USA Getting a grip on anisotropy of the earth can mean the difference between success and failure in reservoir evaluation and development. Accounting for the affects of anisotropy in measurements of the earth begins with understanding the geologic foundations of anisotropy—how sediments are laid down, converted to rock and deformed. Here is a summary of some geologic mechanisms for anisotropy, and some recent progress on anisotropy of electrical properties of rock formations. Across the many disciplines of the oil field, a power now allow anisotropy to be factored stock exchange. A smart one will figure out nearly universal phenomenon is anisotropy into field development decisions. A full how to survive, but not without a struggle. —the variation of a property with the direction mathematical description of anisotropy Physicists first met this challenge early in in which it is measured. Where anisotropy remains difficult—for example, representing this century when they left the laboratory to arises, convenient assumptions fall. Seismic flow in three dimensions requires six vari- make measurements of the earth’s subsur- reflectors appear at the wrong depth. Seismic ables.1 But accounting for the simplest face. They brought with them the mathe- lines don’t tie. Waterflood programs fail. effects of anisotropy is coming within reach. matics of materials assumed to be Induction logs are misinterpreted and mis- What is meant by anisotropy depends on isotropic—having properties with the same take water for pay.
    [Show full text]